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59. Spectral observations of solar activity at metre wave-lengths

Published online by Cambridge University Press:  14 August 2015

J. P. Wild*
Affiliation:
Radiophysics Laboratory, Sydney, Australia

Extract

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This paper summarizes some recent results obtained with the solar radio-spectroscope at Dapto (Sydney), which has been in operation since 1952. The basic instrument is a receiver which sweeps through the frequency range 40–240 Mc./s. every half a second. Each spectrum is displayed as an intensity-modulated line, and successive spectra are recorded photographically on continuously moving film to give a dynamic record of the spectrum.

Type
Part V: The Active Sun
Copyright
Copyright © Cambridge University Press 1957 

References

Wild, J. P. and McCready, L. L. Aust. J. Sci. Res. A , 3, 387, 1950.Google Scholar
Wild, J. P., Murray, J. D. and Rowe, W. C. Aust. J. Phys. 7, 439, 1954.Google Scholar
Wild, J. P., Roberts, J. A. and Murray, J. D. Nature , 173, 532, 1954.Google Scholar